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Solar system, age

Fig. 8.2. Iron content as a function of the age of stars in the neighbourhood of the Solar System (age-metallicity relation). Age determinations are a dehcate matter and somewhat uncertain. This explains the wide error bars and scatter of the data. Type la supernovas must be included to reproduce the observed iron evolution. Fig. 8.2. Iron content as a function of the age of stars in the neighbourhood of the Solar System (age-metallicity relation). Age determinations are a dehcate matter and somewhat uncertain. This explains the wide error bars and scatter of the data. Type la supernovas must be included to reproduce the observed iron evolution.

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